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名稱Title
2018天文年會
國立金門大學
5月18日至20日

論文摘要

Modeling the Magnetic Field Structure Of Molecular Clouds Through Dust Polarization

[ Poster PS22 ]

Yu-Hsuan Hwang (National Taiwan University); Shih-Ping Lai (National Tsing Hua University)

Whether the magnetic field plays an important role during the process of gravitational collapse in the most early stages of low mass protostars is still under debate. It is claimed that there would be an hourglass-characterized magnetic field if the magnetic field affects the process of collapse. NGC1333 IRAS 4A is a famous Class 0 protostar with hourglass morphology, and in this study, we would like to analyze the three dimensional structure of this target by simulating the observational results.